Aquarius II
| Aquarius ll | |
|---|---|
| Observation data | |
| Constellation | Aquarius |
| Distance | 180,000 ly |
| Characteristics | |
| Size | 160 pc |
| Notable features | Difficult detection |
| Other designations | |
| Aquarius 2, AQU 2, Aqu ll | |
Aquarius ll (also Aquarius 2, AQU 2 or Aqu ll) is a mildly elliptical dwarf satellite galaxy to the Milky Way located around 110 kiloparsecs from Earth in the constellation of Aquarius. It has a size of 160 parsecs. Aquarius ll is currently moving away from the galactic center of the Milky Way. This galaxy contains many old red giant branch stars that are predominantly metal poor.
It is located just 9 kiloparsecs from the Large Magellanic Cloud (LMC). Whether this is an association or coincidence is uncertain. Other dwarf galaxies discovered likely do have some association with the Magellanic Clouds.